Hubble Reveals 'Cat's Tail' Dust Cloud Around Beta Pictoris, Offering Insights into Early Solar Systems
New observations from the Hubble Space Telescope have provided a clearer picture of the 'Cat's Tail,' a trail of soot-dark dust around the young star Beta Pictoris, located 63 light-years away. The study, led by University of Arizona doctoral student Arin Avsar, indicates that this dust structure lies mostly flat against the sky from Earth's perspective and is composed almost entirely of porous, carbon-rich grains. These grains are believed to have formed from a collision between two Pluto-sized bodies. The Cat's Tail was initially discovered in 2024 by NASA's James Webb Space Telescope, which detected it in mid-infrared light. Hubble's visible-light images, combined with Webb's infrared data and computer modeling, helped reconstruct the tail's three-dimensional arrangement, revealing its flat orientation and fluffy, carbon-rich composition.